Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars
- Autores
- Longland, Richard; Loren Aguilar, P.; Jose, J.; Garcia Berro, E.; Althaus, Leandro Gabriel; Isern, J.
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Many hydrogen-deficient stars are characterized by surface abundance patterns that are hard to reconcile with conventional stellar evolution. Instead, it has been suggested that they may represent the result of a merger episode between a helium and a carbon-oxygen white dwarf. In this Letter, we present a nucleosynthesis study of the merger of a 0.4 M ☉ helium white dwarf with a 0.8 M ☉ carbon-oxygen white dwarf, by coupling the thermodynamic history of Smoothed Particle Hydrodynamics particles with a post-processing code. The resulting chemical abundance pattern, particularly for oxygen and fluorine, is in qualitative agreement with the observed abundances in R Coronae Borealis stars.
Fil: Longland, Richard. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España
Fil: Loren Aguilar, P.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España
Fil: Jose, J.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España
Fil: Garcia Berro, E.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España
Fil: Althaus, Leandro Gabriel. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina
Fil: Isern, J.. Institut de Ciencies de l’Espai; España. Institut d’Estudis Espacials de Catalunya; España - Materia
-
Nuclear Reactions
Nucleosynthesis
Agb Stars
White Dwarfs - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/10281
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Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis starsLongland, RichardLoren Aguilar, P.Jose, J.Garcia Berro, E.Althaus, Leandro GabrielIsern, J.Nuclear ReactionsNucleosynthesisAgb StarsWhite Dwarfshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Many hydrogen-deficient stars are characterized by surface abundance patterns that are hard to reconcile with conventional stellar evolution. Instead, it has been suggested that they may represent the result of a merger episode between a helium and a carbon-oxygen white dwarf. In this Letter, we present a nucleosynthesis study of the merger of a 0.4 M ☉ helium white dwarf with a 0.8 M ☉ carbon-oxygen white dwarf, by coupling the thermodynamic history of Smoothed Particle Hydrodynamics particles with a post-processing code. The resulting chemical abundance pattern, particularly for oxygen and fluorine, is in qualitative agreement with the observed abundances in R Coronae Borealis stars.Fil: Longland, Richard. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; EspañaFil: Loren Aguilar, P.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; EspañaFil: Jose, J.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; EspañaFil: Garcia Berro, E.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; EspañaFil: Althaus, Leandro Gabriel. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; ArgentinaFil: Isern, J.. Institut de Ciencies de l’Espai; España. Institut d’Estudis Espacials de Catalunya; EspañaIop Publishing2011-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/10281Longland, Richard; Loren Aguilar, P.; Jose, J.; Garcia Berro, E.; Althaus, Leandro Gabriel; et al.; Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars; Iop Publishing; Astrophysical Journal; 737; 8-2011; 34-370004-637Xenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/737/2/L34info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/2041-8205/737/2/L34/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:14:39Zoai:ri.conicet.gov.ar:11336/10281instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:14:39.691CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars |
title |
Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars |
spellingShingle |
Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars Longland, Richard Nuclear Reactions Nucleosynthesis Agb Stars White Dwarfs |
title_short |
Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars |
title_full |
Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars |
title_fullStr |
Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars |
title_full_unstemmed |
Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars |
title_sort |
Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars |
dc.creator.none.fl_str_mv |
Longland, Richard Loren Aguilar, P. Jose, J. Garcia Berro, E. Althaus, Leandro Gabriel Isern, J. |
author |
Longland, Richard |
author_facet |
Longland, Richard Loren Aguilar, P. Jose, J. Garcia Berro, E. Althaus, Leandro Gabriel Isern, J. |
author_role |
author |
author2 |
Loren Aguilar, P. Jose, J. Garcia Berro, E. Althaus, Leandro Gabriel Isern, J. |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Nuclear Reactions Nucleosynthesis Agb Stars White Dwarfs |
topic |
Nuclear Reactions Nucleosynthesis Agb Stars White Dwarfs |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Many hydrogen-deficient stars are characterized by surface abundance patterns that are hard to reconcile with conventional stellar evolution. Instead, it has been suggested that they may represent the result of a merger episode between a helium and a carbon-oxygen white dwarf. In this Letter, we present a nucleosynthesis study of the merger of a 0.4 M ☉ helium white dwarf with a 0.8 M ☉ carbon-oxygen white dwarf, by coupling the thermodynamic history of Smoothed Particle Hydrodynamics particles with a post-processing code. The resulting chemical abundance pattern, particularly for oxygen and fluorine, is in qualitative agreement with the observed abundances in R Coronae Borealis stars. Fil: Longland, Richard. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España Fil: Loren Aguilar, P.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España Fil: Jose, J.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España Fil: Garcia Berro, E.. Universidad Politecnica de Catalunya; España. Institut d’Estudis Espacials de Catalunya; España Fil: Althaus, Leandro Gabriel. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina Fil: Isern, J.. Institut de Ciencies de l’Espai; España. Institut d’Estudis Espacials de Catalunya; España |
description |
Many hydrogen-deficient stars are characterized by surface abundance patterns that are hard to reconcile with conventional stellar evolution. Instead, it has been suggested that they may represent the result of a merger episode between a helium and a carbon-oxygen white dwarf. In this Letter, we present a nucleosynthesis study of the merger of a 0.4 M ☉ helium white dwarf with a 0.8 M ☉ carbon-oxygen white dwarf, by coupling the thermodynamic history of Smoothed Particle Hydrodynamics particles with a post-processing code. The resulting chemical abundance pattern, particularly for oxygen and fluorine, is in qualitative agreement with the observed abundances in R Coronae Borealis stars. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011-08 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/10281 Longland, Richard; Loren Aguilar, P.; Jose, J.; Garcia Berro, E.; Althaus, Leandro Gabriel; et al.; Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars; Iop Publishing; Astrophysical Journal; 737; 8-2011; 34-37 0004-637X |
url |
http://hdl.handle.net/11336/10281 |
identifier_str_mv |
Longland, Richard; Loren Aguilar, P.; Jose, J.; Garcia Berro, E.; Althaus, Leandro Gabriel; et al.; Nucleosynthesis during the merger of white dwarfs and the origin of R Coronae Borealis stars; Iop Publishing; Astrophysical Journal; 737; 8-2011; 34-37 0004-637X |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/737/2/L34 info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/2041-8205/737/2/L34/meta |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Iop Publishing |
publisher.none.fl_str_mv |
Iop Publishing |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844614076234203136 |
score |
13.070432 |